Astronomical, Atmospheric, and Wavefront Studies with a Submillimeter-wavelength Interferometer
Over the course of the last half century, astrophysical investigations have expanded into ever wider sections of the electromagnetic spectrum. One of the most difficult wavebands to access, both for atmospheric and technological reasons, is the submillimeter band, between wavelengths of roughly 1 mm and 100 fim. Home to a large set of molecular rotational transitions [1,2], these wavelengths mark the boundary between radio and infrared waves, and in terms of the atmosphere, coincide with the transition between the high-transparency radio ‘windows’ and the opaque far-infrared sky (Fig. 55.1).
KeywordsMicrowave Hydride Photolysis Boulder Phosphine
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